Nuclear Structure Studies of Neutron-Rich Nuclei : Astrophysical Implications

Abstract : It is proposed here to investigate three major properties of the nuclear force that influence the amplitude of shell gaps, the nuclear binding energies as well as the nuclear $\beta$-decay properties far from stability, that are all key ingredients for modeling the r-process nucleosynthesis. These properties are derived from experiments performed in different facilities worldwide, using several various state-of-the-art experimental techniques including transfer and knockout reactions. Expected consequences on the r process nucleosynthesis as well as on the stability of super heavy elements are discussed.
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Communication dans un congrès
14th International Symposium on Nuclei in the Cosmos (NIC-XIV), Jun 2016, Niigata, Japan. JPS Conference Proceedings, 14, pp.010601, 2017, 〈http://nic2016.jp/〉. 〈10.7566/JPSCP.14.010601〉
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Soumis le : jeudi 5 janvier 2017 - 14:53:48
Dernière modification le : jeudi 1 février 2018 - 01:35:58
Document(s) archivé(s) le : jeudi 6 avril 2017 - 12:26:19

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O. Sorlin. Nuclear Structure Studies of Neutron-Rich Nuclei : Astrophysical Implications. 14th International Symposium on Nuclei in the Cosmos (NIC-XIV), Jun 2016, Niigata, Japan. JPS Conference Proceedings, 14, pp.010601, 2017, 〈http://nic2016.jp/〉. 〈10.7566/JPSCP.14.010601〉. 〈in2p3-01336856〉

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